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  • 1
    Electronic Resource
    Electronic Resource
    Solar rotation in the chromosphere and corona (1973)
    Springer
    Solar physics 33 (1973), S. 425-429 
    Details
    ISSN: 1573-093X
    Source: Springer Online Journal Archives 1860-2000
    Topics: Physics
    Notes: Abstract Extreme ultraviolet spectroheliograms in Mg x (625 Å) and the Lyman continuum (897 Å) obtained from OSO-6 are used to determine the differential rotation rate in the solar chromosphere and corona. The equatorial rotation rate agrees with spectroscopic measurements of the photospheric plasma velocity; the variation of rate with latitude is less pronounced than in most other determinations. We cannot discern a variation in the rotation rate between the chromosphere and corona.
    Type of Medium: Electronic Resource
    URL: http://dx.doi.org/10.1007/BF00152429
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